Amazing Light pp 585-595 | Cite as

Astronomical, Atmospheric, and Wavefront Studies with a Submillimeter-wavelength Interferometer

  • Eugene Serabyn


Over the course of the last half century, astrophysical investigations have expanded into ever wider sections of the electromagnetic spectrum. One of the most difficult wavebands to access, both for atmospheric and technological reasons, is the submillimeter band, between wavelengths of roughly 1 mm and 100 fim. Home to a large set of molecular rotational transitions [1,2], these wavelengths mark the boundary between radio and infrared waves, and in terms of the atmosphere, coincide with the transition between the high-transparency radio ‘windows’ and the opaque far-infrared sky (Fig. 55.1).


Brightness Temperature Rotational Transition Atmospheric Transmission Fourier Transform Spectrometer Water Vapor Column 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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© Springer-Verlag New York, Inc. 1996

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  • Eugene Serabyn

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